γ Cassiopeiae: An X-ray Be star with personality

Astronomy and Astrophysics

Volumn 512, Issue 4, 2010, Pages

  De Oliveira, R Lopes ^a   Smith, M A ^b   Motch, C ^c  

^a UNIVERSITY OF SÃO PAULO   (Brazil)

^b CATHOLIC UNIVERSITY OF AMERICA   (United States)

^c UNIVERSITÉ DE STRASBOURG   (France)

Author keywords

Be; Stars: emission line; Stars: individual: Cas; X rays: stars

Indexed keywords

ABSORPTION SPECTROSCOPY; GAS ABSORPTION; IONS; NEON; PHOTOELECTRICITY; X RAYS;

BE STARS; CHANDRA; EARLY-TYPE - STARS; HIGH DISPERSION; HIGH ENERGY PROCESS; HOT COMPONENTS; K-SHELLS; L SHELL; LIGHT CURVES; MASSIVE STARS; NONTHERMAL EMISSION; PHOTOELECTRIC ABSORPTION; PHYSICAL MECHANISM; SOFT X-RAY; STARS: INDIVIDUAL; THERMAL COMPONENT; THERMAL X-RAYS; TIME-SCALES; UNSOLVED PROBLEMS; X RAYS: STARS; XMM-NEWTON;

STARS;

EID: 77951523623     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811319     Document Type: Article

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